ALMA Discovers Interstellar Comet 3I/ATLAS Originated in a Frigid Planetary System

Water consists of two hydrogen atoms and one oxygen atom, represented as H2O. However, in a standard water molecule, those hydrogen atoms contain only a single proton. In contrast, cometary water features a significant proportion of deuterium (D), a form of hydrogen combining a standard proton with a neutron. This deuterated water, such as that found in the interstellar comet 3I/ATLAS, presents evidence of remarkably different environmental conditions from billions of years ago, akin to the half-heavy water (HDO) identified in comets within our solar system.

This image from the Subaru Telescope shows the interstellar comet 3I/ATLAS. Image provided by: National Astronomical Observatory of Japan

Water is an essential molecule pivotal to life and various astrophysical processes.

From an astrobiological standpoint, water serves as a crucial solvent facilitating the emergence of life on Earth, and it is tracked across the universe as a potential indicator of habitable environments beyond our solar system.

During the formation of stars and planets, water in its gaseous phase acts as an efficient coolant, assisting the collapse of molecular clouds and the birth of stars.

In frozen conditions, water coats dust particles, enhancing their adhesion and accelerating planetary core growth.

Water has been identified in both gaseous and icy forms throughout our galaxy and beyond, even in high-redshift galaxies.

These discoveries encompass the entire solar system, including molecular clouds, protostellar systems, prestellar nuclei, protoplanetary disks, comets, meteorites, active asteroids, planets, and moons.

Current research endeavors aim to link water pathways across these varied environments, aiming to unravel the origins and evolution of water in planetary system formation.

The deuterium-to-hydrogen (D/H) ratio in water acts as a potent chemical tracer, informing where the water was formed, the physical conditions during its creation, and its subsequent treatment.

“Recent observations from the Atacama Large Millimeter/Submillimeter Array (ALMA) indicate that the conditions that led to the formation of our Solar System differ significantly from those that shaped planetary systems in other regions of the Galaxy,” explained Dr. Luis E. Salazar Manzano, a student at the University of Michigan.

“Most instruments can’t survey the sun, but radio telescopes like ALMA can,” Dr. Teresa Paneque Carreño from the University of Michigan added. “We successfully observed the comet just as it passed behind the Sun, shortly after its perihelion.”

“This provides us with constraints on these molecules that other instruments cannot match.”

ALMA’s measurements of the D/H ratio in water from 3I/ATLAS indicate values over 30 times higher than those observed in comets formed within our solar system, and more than 40 times the levels found in Earth’s oceans.

“We’ve established that the gas cloud that birthed the star associated with 3I/ATLAS and the other planets in its system originated under distinct, frigid conditions, contrasting sharply with the environment that formed our solar system and local comets,” Salazar Manzano revealed.

This finding offers a unique fundamental insight, unlike other more complex molecular studies in interstellar comets, as the deuterium-to-hydrogen proportions were determined during the Big Bang.

“The chemical processes leading to deuterium water enrichment are highly temperature-sensitive, typically requiring environments below about 30 K (equivalent to -243 degrees Celsius or -406 degrees Fahrenheit),” Salazar Manzano stated.

The D/H ratio of water in this comet was enriched compared to the Big Bang baseline while it formed and was preserved during its interstellar journey.

This interstellar comet likely formed under very specific radiation conditions in a far colder environment than the history of our solar system before being ejected into interstellar space.

“Each interstellar comet carries fragments of its history and ‘fossils’ from diverse locations,” expressed Dr. Paneque Carreño.

“While the exact formation site remains elusive, instruments like ALMA enable us to begin comprehending the conditions there and drawing comparisons to our solar system.”

The research team’s results were published on April 23rd in the journal Nature Astronomy.

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LE Salazar Manzano et al. 3I/ATLAS water D/H as a probe of another planetary system’s formation status. Nat Astron published online on April 23, 2026. doi: 10.1038/s41550-026-02850-5

Source: www.sci.news

Our Solar System passed through a frigid interstellar cloud approximately 2 million years ago, new research reveals.

A cold, dense cloud in the Milky Way’s interstellar medium is about four to five orders of magnitude denser than its diffuse counterparts, and a team of astronomers from Boston University, Harvard University, and Johns Hopkins University has found evidence that two to three million years ago, our solar system encountered one of these dense clouds, which may have been so dense that it disrupted the solar wind.



Offers othersThe interstellar material through which the Sun has traveled over the past few million years indicates the presence of cold, dense clouds that could have had dramatic effects on the heliosphere. Image credit: NASA/JPL-Caltech.

Most stars generate winds that move through the surrounding interstellar medium.

This motion creates a cocoon that protects the planet from interstellar material. The Sun’s cocoon is the heliosphere.

It’s made up of a constant stream of charged particles called the solar wind, which extends far beyond Pluto, enveloping the planet in what astronomers call a “local bubble.”

It protects us from radiation and galactic rays that can alter DNA, and scientists think it’s part of the reason why life on Earth evolved.

A cold interstellar cloud compressed the heliosphere, temporarily placing Earth and other planets in the solar system outside of its influence, according to a new study.

“Our paper is the first to quantitatively show that there was an encounter between the Sun and something outside our solar system that affected Earth’s climate,” said Professor Merab Auffar of Boston University.

“Stars move, and this paper shows that not only do they move, but they undergo dramatic changes.”

To study this phenomenon, Professor Orpher and his colleagues essentially went back in time and used advanced computer models to visualize where the Sun was located two million years ago, along with the heliosphere and the rest of the solar system.

They also mapped the path of a “localized cold cloud ribbon” system, a series of large, dense and very cold clouds made mainly of hydrogen atoms.

Their simulations showed that one of the clouds near the edge of the ribbon, a “local cold cloud,” may have collided with the heliosphere.

If this had happened, Earth would have been fully exposed to interstellar matter, where gases and dust would have mixed with atomic elements left over from the exploded star, such as iron and plutonium.

Normally, the heliosphere filters out most of these radioactive particles, but without protection they could easily reach Earth.

This is consistent with geological evidence showing increased levels of the isotopes iron-60 and plutonium-244 in the oceans, the moon, Antarctic snow and ice cores from the same period, according to the paper.

This timing also coincides with temperature records indicating a cold period.

“It is rare for our cosmic neighbors outside our solar system to have an impact on life on Earth,” said Harvard University professor Avi Loeb.

“It’s exciting to discover that our passage through dense clouds millions of years ago may have exposed the Earth to much greater amounts of cosmic rays and atomic hydrogen.”

“Our findings open a new window into the evolution of life on Earth and its relationship with our cosmic neighbours.”

“External pressure from localized lynxes of cold clouds could have continuously blocked the heliosphere for hundreds to millions of years, depending on the size of the cloud.”

“But as soon as Earth left the cold cloud, the heliosphere engulfed all the planets, including Earth.”

“It’s impossible to know exactly what effect the cold clouds had on the Earth, such as whether they caused ice ages.”

“But there are other cool clouds in the interstellar medium that the Sun likely encountered in its first few billion years.”

“And we’ll probably encounter many more over the next million years or so.”

The authors are currently working to determine where the Sun was 7 million years ago, and beyond.

Pinpointing the position of the Sun and cold cloud systems millions of years ago is made possible by data collected by ESA’s Gaia mission, which has produced the largest 3D map of the galaxy ever, showing in unprecedented detail how fast stars move.

“This cloud is certainly from our past, and if we passed through something this massive, we would have been exposed to interstellar material,” Prof Auffar said.

“This is just the beginning. We hope this paper opens the door to further exploration of how the solar system was influenced by outside forces in the ancient past, and how these forces may have shaped life on Earth.”

of paper Published in today’s journal Natural Astronomy.

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M. Offer othersIt is possible that Earth was directly exposed to cold, dense interstellar material 2 to 3 million years ago. Nat AstronPublished online June 10, 2024; doi: 10.1038/s41550-024-02279-8

Source: www.sci.news